aoflagger 3.1.0-2build4 source package in Ubuntu
Changelog
aoflagger (3.1.0-2build4) kinetic; urgency=medium * No-change rebuild against libcasa-casa7 -- Steve Langasek <email address hidden> Sat, 16 Jul 2022 17:50:58 +0000
Upload details
- Uploaded by:
- Steve Langasek
- Uploaded to:
- Kinetic
- Original maintainer:
- Ubuntu Developers
- Architectures:
- any
- Section:
- misc
- Urgency:
- Medium Urgency
See full publishing history Publishing
Series | Published | Component | Section |
---|
Downloads
File | Size | SHA-256 Checksum |
---|---|---|
aoflagger_3.1.0.orig.tar.gz | 978.3 KiB | 86a83cd8b90bde24d8c9533cbccdfddc9d3b2ed9cc74f082456bc1a975883e60 |
aoflagger_3.1.0-2build4.debian.tar.xz | 9.3 KiB | 99d6c56cffc4cd6cddd7c65980b58f9f2b7e6674d077911c88990745f2464a8a |
aoflagger_3.1.0-2build4.dsc | 2.5 KiB | 2bdac4ea7df07d0fdb22bc476ff8e1cea5d339b070eb313879d3b123c3e1786b |
Available diffs
- diff from 3.1.0-2build3 to 3.1.0-2build4 (330 bytes)
Binary packages built by this source
- aoflagger: No summary available for aoflagger in ubuntu kinetic.
No description available for aoflagger in ubuntu kinetic.
- aoflagger-dbgsym: debug symbols for aoflagger
- aoflagger-dev: Find RFI in radio astronomical observations (development files)
The AOFlagger is a tool that can find and remove radio-frequency interference
(RFI) in radio astronomical observations. The code has been highly optimized
for speed and accuracy. It is used by default for the LOFAR radio telescope
and thus is in productional stage. The software can run in a fully automated
way, but a graphical interface is provided to analyse results and tweak the
strategy. The preferred input file format is the Casa Measurement Set (MS)
format.
.
This package contains the header file to compile own programs against
the library.
- libaoflagger0: Find RFI in radio astronomical observations (shared lib)
The AOFlagger is a tool that can find and remove radio-frequency interference
(RFI) in radio astronomical observations. The code has been highly optimized
for speed and accuracy. It is used by default for the LOFAR radio telescope
and thus is in productional stage. The software can run in a fully automated
way, but a graphical interface is provided to analyse results and tweak the
strategy. The preferred input file format is the Casa Measurement Set (MS)
format.
.
This package contains the shared library.
- libaoflagger0-dbgsym: No summary available for libaoflagger0-dbgsym in ubuntu kinetic.
No description available for libaoflagger0-
dbgsym in ubuntu kinetic.